C            *****    JPL Planetary and Lunar Ephemerides    *****
C
C                                      Version : August 28, 2007
C
C     Program TESTEPH
C     ---------------
C  
C     TESTEPH tests the JPL ephemeris reading and interpolating routine using
C     examples computed from the original ephemeris.
C
C     TESTEPH contains the reading and interpolating subroutines that are of 
C     eventual interest to the user.  Once TESTEPH is working correctly, the 
C     user can extract those subroutines and the installation process is complete.
C
C     You must supply "testpo.XXX" to TESTEPH, via standard input.  "testpo.XXX
C     is the specially formatted text file that contains the test cases for the 
C     ephmeris, DEXXX.
C
C     After the initial identifying text which is concluded by an "EOT" in
C     columns 1-3, the test file contains the following quantities:
C
C         JPL Ephemeris Number
C         calendar date
C         Julian Ephemeris Date
C         target number (1-Mercury, ...,3-Earth, ,,,9-Pluto, 10-Moon, 11-Sun,
C                        12-Solar System Barycenter, 13-Earth-Moon Barycenter
C                        14-Nutations, 15-Librations)
C         center number (same codes as target number)
C         coordinate number (1-x, 2-y, ... 6-zdot) 
C         coordinate  [au, au/day]
C
C     For each test case input, TESTEPH
C
C         - computes the corresponding state from data contained 
C           in DExxx,
C
C         - compares the two sets,
C
C         - writes an error message if the difference between
C           any of the state components is greater than 10**(-13).
C
C         - writes state and difference information for every 100th
C           test case processed.
C
C
C      This program is written in standard Fortran-77.  
C
C      HOWEVER, there are two parts which are compiler dependent; both have
C      to do with opening and reading a direct-access file.  They are dealt
C      with in the subroutine FSIZERi, i=1,3.  (There are three versions of 
C      this subroutine.
C
C      1) The parameter RECL in the OPEN statement is the number of units per 
C         record.  For some compilers, it is given in bytes; in some, it is given
C         in single precision words.  In the subroutine FSIZER of TESTEPH, the
C         parameter NRECL must be set to 4 if RECL is given in bytes; NRECL must 
C         be set to 1 if RECL is given in words.  (If in doubt, use 4 for UNIX;
C         1 for VAX and PC)
C
C      2) Also for the OPEN statement, the program needs to know the exact value
C         of RECL (number of single precision words times NRECL).  Since this 
C         varies from one JPL ephemeris to another, RECL must be determined somehow 
C         and given to the OPEN statement.  There are three methods, depending 
C         upon the compiler.  We have included three versions of the subroutine 
C         FSIZER, one for each method.
C
C         a)  Use the INQUIRE statement to find the length of the records 
C             automatically before opening the file.  This works for VAX's; 
C             not in UNIX.
C
C         b)  Open the file with an arbitrary value of RECL, read the first record,
C             and use the information on that record to determine the exact value
C             of RECL.  Then, close the file and re-open it with the exact value.
C             This seems to work for UNIX compilers as long as the initial value of
C             RECL is less than the exact value but large enough to get the required 
C             information from the first file.  (For other compilers, this doesn't
C             work since you can open a file only with the exact value of RECL.)
C
C         c)  Hardwire the value of RECL.  This number is NRECL*1652 for DE200, 
C             NRECL*2036 for DE405, and NRECL*1456 for DE406.
C
C             
C
       subroutine aaa()

       CHARACTER*6  NAMS(400)
       CHARACTER*3  ALF3

       DOUBLE PRECISION  DEL
       DOUBLE PRECISION  ET
       DOUBLE PRECISION  R(6)
       DOUBLE PRECISION  SS(3)
       DOUBLE PRECISION  VALS(400)
       DOUBLE PRECISION  XI
  
       INTEGER  I
       INTEGER  LINE
       data line/0/
       INTEGER  NVS,NTARG,NCTR,NCOORD
       INTEGER  NPT
       data npt/100/

C      Write a fingerprint to the screen.

       WRITE(*,*) ' JPL TEST-EPHEMERIS program. ' //
     .            ' Last modified August 28, 2007.'

C      Print the ephemeris constants.

       CALL  Const (NAMS, VALS, SS, NVS)

       WRITE (*,'(/3F14.2/200(/2(A8,D24.16)))') SS,
     .                                         (NAMS(I),VALS(I),I=1,NVS)

C     Skip the file header comments.

   1  READ(*,'(a3)')ALF3
      IF(ALF3 .NE. 'EOT') GO TO 1

      WRITE(*,*) 
     . '  line -- jed --   t#   c#   x#   --- jpl value ---'//
     . '   --- user value --    -- difference --'
      WRITE(*,*) 

C     Read a value from the test case; skip if not within the time-range
C     of the present version of the ephemeris

   2  READ(*,'(15X,D10.1,3I3,F30.20)',END=9)  
     . ET,NTARG,NCTR,NCOORD,XI

CCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCC

C  NOTE : Over the years, different versions of PLEPH have had a fifth argument:
C  sometimes, an error return statement number; sometimes, a logical denoting
C  whether or not the requested date is covered by the ephemeris.  We apologize
C  for this inconsistency; in this version, we use only the four necessary 
C  arguments and do the testing outside of the subroutine.

      IF(ET .LT. SS(1)) GO TO 2
      IF(ET .GT. SS(2)) GO TO 2

      CALL  Pleph ( ET, NTARG, NCTR, R )

CCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCC

c     For testing purposes DEL is the computation of the difference in
c       read values of the ephemeris converted from the export ascii files
c       versus those printed form the original integration.
c     The difference is checked for random parameters, one every 32 day interval.
c     The agreement is considered okay if DEl is less that 1e-13.
c     This corresponds to a few cm for body positions, and very small
c     values for velocities, and angles and their rates.
c       (A fractional test isn't suitable since sometimes the values will
c        be near zero for parituclar components.)
c     For lunar libration psi, NCOORD=15, the angle accumulates in time
c     so precision is lost after several centuries. This is handled below
c     by scaling DEL down for psi and d(psi)/dt, as opposed to having differnt
c     tolerances for different types of quantities.

      DEL=DABS(R(NCOORD)-XI)

      if(ntarg .eq. 15 .and. ncoord .eq. 3)then
        del=del/(0.23d0*(et-2451545.d0))
      endif
      if(ntarg .eq. 15 .and. ncoord .eq. 6)then
        del=del*0.01/(1.0d0+(et-2451545.d0)/365.25e2)
      endif

      LINE=LINE+1

      IF ( MOD(LINE,npt) .EQ. 0 )  WRITE(*,200)
     . LINE,ET,NTARG,NCTR,NCOORD,XI,R(NCOORD),DEL
 200  FORMAT(I6,F10.1,3I5,2F25.13,1E13.5)

C  Print out WARNING if difference greater than tolerance.
C
      IF (DEL .GE. 1.D-13) WRITE(*,201) 
     . LINE,ET,NTARG,NCTR,NCOORD,XI,R(NCOORD),DEL
 201  FORMAT(/ '*****  WARNING : next difference >= 1.D-13  *****'//
     . I6,F10.1,3I3,2F25.13,1E13.5/' ')

      GO TO 2

   9  STOP
      END
      


C++++++++++++++++++++++++
C
      SUBROUTINE FSIZER1(NRECL,KSIZE,NRFILE,NAMFIL)
C
C++++++++++++++++++++++++
C
C   Version 1.0 uses the INQUIRE statement to find out the the record length 
C   of the direct access file before opening it.  This procedure is non-standard, 
C   but seems to work for VAX machines. 
C
C  THE SUBROUTINE ALSO SETS THE VALUES OF  NRECL, NRFILE, AND NAMFIL.

C  *****************************************************************
C  *****************************************************************
C
C  THE PARAMETERS NAMFIL, NRECL, AND NRFILE ARE TO BE SET BY THE USER
C
C  *****************************************************************

C  NAMFIL IS THE EXTERNAL NAME OF THE BINARY EPHEMERIS FILE

      CHARACTER*80  NAMFIL

      NAMFIL="de421.dos"

C  *****************************************************************

C  NRECL=1 IF "RECL" IN THE OPEN STATEMENT IS THE RECORD LENGTH IN S.P. WORDS
C  NRECL=4 IF "RECL" IN THE OPEN STATEMENT IS THE RECORD LENGTH IN BYTES
C  (for a VAX, it is probably 1)
C
      NRECL= 4

C  *****************************************************************

C  NRFILE IS THE INTERNAL UNIT NUMBER USED FOR THE EPHEMERIS FILE

      NRFILE=12

C  *****************************************************************

C   FIND THE RECORD SIZE USING THE INQUIRE STATEMENT  


      IRECSZ=0

      INQUIRE(FILE=NAMFIL,RECL=IRECSZ)

C IF 'INQUIRE' DOES NOT WORK, USUALLY IRECSZ WILL BE LEFT AT 0 

      IF(IRECSZ .LE. 0) write(*,*)
     . ' INQUIRE STATEMENT PROBABLY DID NOT WORK'

      KSIZE=IRECSZ/NRECL

      RETURN

      END
C++++++++++++++++++++++++
C
      SUBROUTINE FSIZER2(NRECL,KSIZE,NRFILE,NAMFIL)
C
C++++++++++++++++++++++++
C  THIS SUBROUTINE OPENS THE FILE, 'NAMFIL', WITH A PHONY RECORD LENGTH, READS 
C  THE FIRST RECORD, AND USES THE INFO TO COMPUTE KSIZE, THE NUMBER OF SINGLE 
C  PRECISION WORDS IN A RECORD.  
C
C  THE SUBROUTINE ALSO SETS THE VALUES OF  NRECL, NRFILE, AND NAMFIL.

      IMPLICIT DOUBLE PRECISION(A-H,O-Z)

      SAVE

      CHARACTER*6 TTL(14,3),CNAM(400)
      CHARACTER*80 NAMFIL

      DIMENSION SS(3)

      INTEGER IPT(3,13)
	  
      CHARACTER*80 EXTNAMFIL
      COMMON/ETHEM_FILE_NAME/EXTNAMFIL

C  *****************************************************************
C  *****************************************************************
C
C  THE PARAMETERS NRECL, NRFILE, AND NAMFIL ARE TO BE SET BY THE USER
C
C  *****************************************************************

C  NRECL=1 IF "RECL" IN THE OPEN STATEMENT IS THE RECORD LENGTH IN S.P. WORDS
C  NRECL=4 IF "RECL" IN THE OPEN STATEMENT IS THE RECORD LENGTH IN BYTES
C  (for UNIX, it is probably 4)
C
      NRECL=4

C  NRFILE IS THE INTERNAL UNIT NUMBER USED FOR THE EPHEMERIS FILE

      NRFILE=12

C  NAMFIL IS THE EXTERNAL NAME OF THE BINARY EPHEMERIS FILE


      NAMFIL=EXTNAMFIL 

C  *****************************************************************
C  *****************************************************************

C  **  OPEN THE DIRECT-ACCESS FILE AND GET THE POINTERS IN ORDER TO 
C  **  DETERMINE THE SIZE OF THE EPHEMERIS RECORD

      MRECL=NRECL*1000

        OPEN(NRFILE,
     *       FILE=NAMFIL,
     *       ACCESS='DIRECT',
     *       FORM='UNFORMATTED',
     *       RECL=MRECL,
     *       STATUS='OLD')

      READ(NRFILE,REC=1)TTL,CNAM,SS,NCON,AU,EMRAT,
     * ((IPT(I,J),I=1,3),J=1,12),NUMDE,(IPT(I,13),I=1,3)

      CLOSE(NRFILE)



C  FIND THE NUMBER OF EPHEMERIS COEFFICIENTS FROM THE POINTERS

      KMX = 0
      KHI = 0

      DO I = 1,13
         IF (IPT(1,I) .GT. KMX) THEN
            KMX = IPT(1,I)
            KHI = I
         ENDIF
      ENDDO

      ND = 3
      IF (KHI .EQ. 12) ND=2

      KSIZE = 2*(IPT(1,KHI)+ND*IPT(2,KHI)*IPT(3,KHI)-1)
	write(*,*) KSIZE
      RETURN

      END
C++++++++++++++++++++++++
C
      SUBROUTINE FSIZER3(NRECL,KSIZE,NRFILE,NAMFIL)
	  
C
C++++++++++++++++++++++++
C
C  THE SUBROUTINE SETS THE VALUES OF  NRECL, KSIZE, NRFILE, AND NAMFIL.

      SAVE

      CHARACTER*80 NAMFIL

C  *****************************************************************
C  *****************************************************************
C
C  THE PARAMETERS NRECL, NRFILE, AND NAMFIL ARE TO BE SET BY THE USER

C  *****************************************************************

C  NRECL=1 IF "RECL" IN THE OPEN STATEMENT IS THE RECORD LENGTH IN S.P. WORDS
C  NRECL=4 IF "RECL" IN THE OPEN STATEMENT IS THE RECORD LENGTH IN BYTES

      NRECL=4

C  *****************************************************************

C  NRFILE IS THE INTERNAL UNIT NUMBER USED FOR THE EPHEMERIS FILE (DEFAULT: 12)

      NRFILE=12

C  *****************************************************************

C  NAMFIL IS THE EXTERNAL NAME OF THE BINARY EPHEMERIS FILE

      NAMFIL="de421.dos" 

C  *****************************************************************

C  KSIZE must be set by the user according to the ephemeris to be read

C  For  de200, set KSIZE to 1652
C  For  de405, set KSIZE to 2036
C  For  de406, set KSIZE to 1456
C  For  de414, set KSIZE to 2036

      KSIZE = 2036

C  *******************************************************************

      RETURN

      END
C++++++++++++++++++++++++++
C
      SUBROUTINE PLEPH ( ET, NTARG, NCENT, RRD )
C
C++++++++++++++++++++++++++
C  NOTE : Over the years, different versions of PLEPH have had a fifth argument:
C  sometimes, an error return statement number; sometimes, a logical denoting
C  whether or not the requested date is covered by the ephemeris.  We apologize
C  for this inconsistency; in this present version, we use only the four necessary 
C  arguments and do the testing outside of the subroutine.
C
C
C
C     THIS SUBROUTINE READS THE JPL PLANETARY EPHEMERIS
C     AND GIVES THE POSITION AND VELOCITY OF THE POINT 'NTARG'
C     WITH RESPECT TO 'NCENT'.
C
C     CALLING SEQUENCE PARAMETERS:
C
C       ET = D.P. JULIAN EPHEMERIS DATE AT WHICH INTERPOLATION
C            IS WANTED.
C
C       ** NOTE THE ENTRY DPLEPH FOR A DOUBLY-DIMENSIONED TIME **
C          THE REASON FOR THIS OPTION IS DISCUSSED IN THE 
C          SUBROUTINE STATE
C
C     NTARG = INTEGER NUMBER OF 'TARGET' POINT.
C
C     NCENT = INTEGER NUMBER OF CENTER POINT.
C
C            THE NUMBERING CONVENTION FOR 'NTARG' AND 'NCENT' IS:
C
C                1 = MERCURY           8 = NEPTUNE
C                2 = VENUS             9 = PLUTO
C                3 = EARTH            10 = MOON
C                4 = MARS             11 = SUN
C                5 = JUPITER          12 = SOLAR-SYSTEM BARYCENTER
C                6 = SATURN           13 = EARTH-MOON BARYCENTER
C                7 = URANUS           14 = NUTATIONS (LONGITUDE AND OBLIQ)
C                            15 = LIBRATIONS, IF ON EPH FILE
C
C             (IF NUTATIONS ARE WANTED, SET NTARG = 14. FOR LIBRATIONS,
C              SET NTARG = 15. SET NCENT=0.)
C
C      RRD = OUTPUT 6-WORD D.P. ARRAY CONTAINING POSITION AND VELOCITY
C            OF POINT 'NTARG' RELATIVE TO 'NCENT'. THE UNITS ARE AU AND
C            AU/DAY. FOR LIBRATIONS THE UNITS ARE RADIANS AND RADIANS
C            PER DAY. IN THE CASE OF NUTATIONS THE FIRST FOUR WORDS OF
C            RRD WILL BE SET TO NUTATIONS AND RATES, HAVING UNITS OF
C            RADIANS AND RADIANS/DAY.
C
C            The option is available to have the units in km and km/sec.
C            For this, set km=.true. in the STCOMX common block.
C

      IMPLICIT DOUBLE PRECISION (A-H,O-Z)

      DIMENSION RRD(6),ET2Z(2),ET2(2),PV(6,13)
      DIMENSION SS(3),CVAL(400),PVSUN(6),zips(2)
      data zips/2*0.d0/

      LOGICAL BSAVE,KM,BARY
      LOGICAL FIRST
      DATA FIRST/.TRUE./

      INTEGER LIST(12),IPT(39),DENUM


      COMMON/EPHHDR/CVAL,SS,AU,EMRAT,DENUM,NCON,IPT

      COMMON/STCOMX/KM,BARY,PVSUN

C     INITIALIZE ET2 FOR 'STATE' AND SET UP COMPONENT COUNT
C
      ET2(1)=ET
      ET2(2)=0.D0
      GO TO 11

C     ENTRY POINT 'DPLEPH' FOR DOUBLY-DIMENSIONED TIME ARGUMENT 
C          (SEE THE DISCUSSION IN THE SUBROUTINE STATE)

      ENTRY DPLEPH(ET2Z,NTARG,NCENT,RRD)

      ET2(1)=ET2Z(1)
      ET2(2)=ET2Z(2)

  11  IF(FIRST) CALL STATE(zips,list,pv,pnut)
      FIRST=.FALSE.

  96  IF(NTARG .EQ. NCENT) RETURN

      DO I=1,12
      LIST(I)=0
      ENDDO

C     CHECK FOR NUTATION CALL

      IF(NTARG.NE.14) GO TO 97
        IF(IPT(35).GT.0) THEN
          LIST(11)=2
          CALL STATE(ET2,LIST,PV,RRD)
          RETURN
        ELSE
          do i=1,4
          rrd(i)=0.d0
          enddo
          WRITE(6,297)
  297     FORMAT(' *****  NO NUTATIONS ON THE EPHEMERIS FILE  *****')
          STOP
        ENDIF

C     CHECK FOR LIBRATIONS

  97  do i=1,6
      rrd(i)=0.d0
      enddo

      IF(NTARG.NE.15) GO TO 98
        IF(IPT(38).GT.0) THEN
          LIST(12)=2
          CALL STATE(ET2,LIST,PV,RRD)
          DO I=1,6
          RRD(I)=PV(I,11)
          ENDDO
          RETURN
        ELSE
          WRITE(6,298)
  298     FORMAT(' *****  NO LIBRATIONS ON THE EPHEMERIS FILE  *****')
          STOP
        ENDIF

C       FORCE BARYCENTRIC OUTPUT BY 'STATE'

  98  BSAVE=BARY
      BARY=.TRUE.

C       SET UP PROPER ENTRIES IN 'LIST' ARRAY FOR STATE CALL

      DO I=1,2
      K=NTARG
      IF(I .EQ. 2) K=NCENT
      IF(K .LE. 10) LIST(K)=2
      IF(K .EQ. 10) LIST(3)=2
      IF(K .EQ. 3) LIST(10)=2
      IF(K .EQ. 13) LIST(3)=2
      ENDDO

C       MAKE CALL TO STATE

      CALL STATE(ET2,LIST,PV,RRD)

      IF(NTARG .EQ. 11 .OR. NCENT .EQ. 11) THEN
      DO I=1,6
      PV(I,11)=PVSUN(I)
      ENDDO
      ENDIF

      IF(NTARG .EQ. 12 .OR. NCENT .EQ. 12) THEN
      DO I=1,6
      PV(I,12)=0.D0
      ENDDO
      ENDIF

      IF(NTARG .EQ. 13 .OR. NCENT .EQ. 13) THEN
      DO I=1,6
      PV(I,13)=PV(I,3)
      ENDDO
      ENDIF

      IF(NTARG*NCENT .EQ. 30 .AND. NTARG+NCENT .EQ. 13) THEN
      DO I=1,6
      PV(I,3)=0.D0
      ENDDO
      GO TO 99
      ENDIF

      IF(LIST(3) .EQ. 2) THEN
      DO I=1,6
      PV(I,3)=PV(I,3)-PV(I,10)/(1.D0+EMRAT)
      ENDDO
      ENDIF

      IF(LIST(10) .EQ. 2) THEN
      DO I=1,6
      PV(I,10)=PV(I,3)+PV(I,10)
      ENDDO
      ENDIF

  99  DO I=1,6
      RRD(I)=PV(I,NTARG)-PV(I,NCENT)
      ENDDO

      BARY=BSAVE

      RETURN
      END
C+++++++++++++++++++++++++++++++++
C
      SUBROUTINE INTERP(BUF,T,NCF,NCM,NA,IFL,PV)
C
C+++++++++++++++++++++++++++++++++
C
C     THIS SUBROUTINE DIFFERENTIATES AND INTERPOLATES A
C     SET OF CHEBYSHEV COEFFICIENTS TO GIVE POSITION AND VELOCITY
C
C     CALLING SEQUENCE PARAMETERS:
C
C       INPUT:
C
C         BUF   1ST LOCATION OF ARRAY OF D.P. CHEBYSHEV COEFFICIENTS OF POSITION
C
C           T   T(1) IS DP FRACTIONAL TIME IN INTERVAL COVERED BY
C               COEFFICIENTS AT WHICH INTERPOLATION IS WANTED
C               (0 .LE. T(1) .LE. 1).  T(2) IS DP LENGTH OF WHOLE
C               INTERVAL IN INPUT TIME UNITS.
C
C         NCF   # OF COEFFICIENTS PER COMPONENT
C
C         NCM   # OF COMPONENTS PER SET OF COEFFICIENTS
C
C          NA   # OF SETS OF COEFFICIENTS IN FULL ARRAY
C               (I.E., # OF SUB-INTERVALS IN FULL INTERVAL)
C
C          IFL  INTEGER FLAG: =1 FOR POSITIONS ONLY
C                             =2 FOR POS AND VEL
C
C
C       OUTPUT:
C
C         PV   INTERPOLATED QUANTITIES REQUESTED.  DIMENSION
C               EXPECTED IS PV(NCM,IFL), DP.
C
C
      IMPLICIT DOUBLE PRECISION (A-H,O-Z)
C
      SAVE
C
      DOUBLE PRECISION BUF(NCF,NCM,*),T(2),PV(NCM,*),PC(18),VC(18)

C
      DATA NP/2/
      DATA NV/3/
      DATA TWOT/0.D0/
      DATA PC(1),PC(2)/1.D0,0.D0/
      DATA VC(2)/1.D0/
C
C       ENTRY POINT. GET CORRECT SUB-INTERVAL NUMBER FOR THIS SET
C       OF COEFFICIENTS AND THEN GET NORMALIZED CHEBYSHEV TIME
C       WITHIN THAT SUBINTERVAL.
C
      DNA=DBLE(NA)
      DT1=DINT(T(1))
      TEMP=DNA*T(1)
      L=IDINT(TEMP-DT1)+1

C         TC IS THE NORMALIZED CHEBYSHEV TIME (-1 .LE. TC .LE. 1)

      TC=2.D0*(DMOD(TEMP,1.D0)+DT1)-1.D0

C       CHECK TO SEE WHETHER CHEBYSHEV TIME HAS CHANGED,
C       AND COMPUTE NEW POLYNOMIAL VALUES IF IT HAS.
C       (THE ELEMENT PC(2) IS THE VALUE OF T1(TC) AND HENCE
C       CONTAINS THE VALUE OF TC ON THE PREVIOUS CALL.)

      IF(TC.NE.PC(2)) THEN
        NP=2
        NV=3
        PC(2)=TC
        TWOT=TC+TC
      ENDIF
C
C       BE SURE THAT AT LEAST 'NCF' POLYNOMIALS HAVE BEEN EVALUATED
C       AND ARE STORED IN THE ARRAY 'PC'.
C
      IF(NP.LT.NCF) THEN
        DO 1 I=NP+1,NCF
        PC(I)=TWOT*PC(I-1)-PC(I-2)
    1   CONTINUE
        NP=NCF
      ENDIF
C
C       INTERPOLATE TO GET POSITION FOR EACH COMPONENT
C
      DO 2 I=1,NCM
      PV(I,1)=0.D0
      DO 3 J=NCF,1,-1
      PV(I,1)=PV(I,1)+PC(J)*BUF(J,I,L)
    3 CONTINUE
    2 CONTINUE
      IF(IFL.LE.1) RETURN
C
C       IF VELOCITY INTERPOLATION IS WANTED, BE SURE ENOUGH
C       DERIVATIVE POLYNOMIALS HAVE BEEN GENERATED AND STORED.
C
      VFAC=(DNA+DNA)/T(2)
      VC(3)=TWOT+TWOT
      IF(NV.LT.NCF) THEN
        DO 4 I=NV+1,NCF
        VC(I)=TWOT*VC(I-1)+PC(I-1)+PC(I-1)-VC(I-2)
    4   CONTINUE
        NV=NCF
      ENDIF
C
C       INTERPOLATE TO GET VELOCITY FOR EACH COMPONENT
C
      DO 5 I=1,NCM
      PV(I,2)=0.D0
      DO 6 J=NCF,2,-1
      PV(I,2)=PV(I,2)+VC(J)*BUF(J,I,L)
    6 CONTINUE
      PV(I,2)=PV(I,2)*VFAC
    5 CONTINUE
C
      RETURN
C
      END

C+++++++++++++++++++++++++
C
      SUBROUTINE SPLIT(TT,FR)
C
C+++++++++++++++++++++++++
C
C     THIS SUBROUTINE BREAKS A D.P. NUMBER INTO A D.P. INTEGER
C     AND A D.P. FRACTIONAL PART.
C
C     CALLING SEQUENCE PARAMETERS:
C
C       TT = D.P. INPUT NUMBER
C
C       FR = D.P. 2-WORD OUTPUT ARRAY.
C            FR(1) CONTAINS INTEGER PART
C            FR(2) CONTAINS FRACTIONAL PART
C
C            FOR NEGATIVE INPUT NUMBERS, FR(1) CONTAINS THE NEXT
C            MORE NEGATIVE INTEGER; FR(2) CONTAINS A POSITIVE FRACTION.
C
C       CALLING SEQUENCE DECLARATIONS
C
      IMPLICIT DOUBLE PRECISION (A-H,O-Z)

      DIMENSION FR(2)

C       MAIN ENTRY -- GET INTEGER AND FRACTIONAL PARTS

      FR(1)=DINT(TT)
      FR(2)=TT-FR(1)

      IF(TT.GE.0.D0 .OR. FR(2).EQ.0.D0) RETURN

C       MAKE ADJUSTMENTS FOR NEGATIVE INPUT NUMBER

      FR(1)=FR(1)-1.D0
      FR(2)=FR(2)+1.D0

      RETURN

      END


C++++++++++++++++++++++++++++++++
C
      SUBROUTINE STATE(ET2,LIST,PV,PNUT)
C
C++++++++++++++++++++++++++++++++
C
C THIS SUBROUTINE READS AND INTERPOLATES THE JPL PLANETARY EPHEMERIS FILE
C
C     CALLING SEQUENCE PARAMETERS:
C
C     INPUT:
C
C         ET2   DP 2-WORD JULIAN EPHEMERIS EPOCH AT WHICH INTERPOLATION
C               IS WANTED.  ANY COMBINATION OF ET2(1)+ET2(2) WHICH FALLS
C               WITHIN THE TIME SPAN ON THE FILE IS A PERMISSIBLE EPOCH.
C
C                A. FOR EASE IN PROGRAMMING, THE USER MAY PUT THE
C                   ENTIRE EPOCH IN ET2(1) AND SET ET2(2)=0.
C
C                B. FOR MAXIMUM INTERPOLATION ACCURACY, SET ET2(1) =
C                   THE MOST RECENT MIDNIGHT AT OR BEFORE INTERPOLATION
C                   EPOCH AND SET ET2(2) = FRACTIONAL PART OF A DAY
C                   ELAPSED BETWEEN ET2(1) AND EPOCH.
C
C                C. AS AN ALTERNATIVE, IT MAY PROVE CONVENIENT TO SET
C                   ET2(1) = SOME FIXED EPOCH, SUCH AS START OF INTEGRATION,
C                   AND ET2(2) = ELAPSED INTERVAL BETWEEN THEN AND EPOCH.
C
C        LIST   12-WORD INTEGER ARRAY SPECIFYING WHAT INTERPOLATION
C               IS WANTED FOR EACH OF THE BODIES ON THE FILE.
C
C                         LIST(I)=0, NO INTERPOLATION FOR BODY I
C                                =1, POSITION ONLY
C                                =2, POSITION AND VELOCITY
C
C               THE DESIGNATION OF THE ASTRONOMICAL BODIES BY I IS:
C
C                         I = 1: MERCURY
C                           = 2: VENUS
C                           = 3: EARTH-MOON BARYCENTER
C                           = 4: MARS
C                           = 5: JUPITER
C                           = 6: SATURN
C                           = 7: URANUS
C                           = 8: NEPTUNE
C                           = 9: PLUTO
C                           =10: GEOCENTRIC MOON
C                           =11: NUTATIONS IN LONGITUDE AND OBLIQUITY
C                           =12: LUNAR LIBRATIONS (IF ON FILE)
C
C
C     OUTPUT:
C
C          PV   DP 6 X 11 ARRAY THAT WILL CONTAIN REQUESTED INTERPOLATED
C               QUANTITIES.  THE BODY SPECIFIED BY LIST(I) WILL HAVE ITS
C               STATE IN THE ARRAY STARTING AT PV(1,I).  (ON ANY GIVEN
C               CALL, ONLY THOSE WORDS IN 'PV' WHICH ARE AFFECTED BY THE
C               FIRST 10 'LIST' ENTRIES (AND BY LIST(12) IF LIBRATIONS ARE
C               ON THE FILE) ARE SET.  THE REST OF THE 'PV' ARRAY
C               IS UNTOUCHED.)  THE ORDER OF COMPONENTS STARTING IN
C               PV(1,I) IS: X,Y,Z,DX,DY,DZ.
C
C               ALL OUTPUT VECTORS ARE REFERENCED TO THE EARTH MEAN
C               EQUATOR AND EQUINOX OF J2000 IF THE DE NUMBER IS 200 OR
C               GREATER; OF B1950 IF THE DE NUMBER IS LESS THAN 200. 
C
C               THE MOON STATE IS ALWAYS GEOCENTRIC; THE OTHER NINE STATES 
C               ARE EITHER HELIOCENTRIC OR SOLAR-SYSTEM BARYCENTRIC, 
C               DEPENDING ON THE SETTING OF COMMON FLAGS (SEE BELOW).
C
C               LUNAR LIBRATIONS, IF ON FILE, ARE PUT INTO PV(K,11) IF
C               LIST(12) IS 1 OR 2.
C
C         NUT   DP 4-WORD ARRAY THAT WILL CONTAIN NUTATIONS AND RATES,
C               DEPENDING ON THE SETTING OF LIST(11).  THE ORDER OF
C               QUANTITIES IN NUT IS:
C
C                        D PSI  (NUTATION IN LONGITUDE)
C                        D EPSILON (NUTATION IN OBLIQUITY)
C                        D PSI DOT
C                        D EPSILON DOT
C
C           *   STATEMENT # FOR ERROR RETURN, IN CASE OF EPOCH OUT OF
C               RANGE OR I/O ERRORS.
C
C
C     COMMON AREA STCOMX:
C
C          KM   LOGICAL FLAG DEFINING PHYSICAL UNITS OF THE OUTPUT
C               STATES. KM = .TRUE., KM AND KM/SEC
C                          = .FALSE., AU AND AU/DAY
C               DEFAULT VALUE = .FALSE.  (KM DETERMINES TIME UNIT
C               FOR NUTATIONS AND LIBRATIONS.  ANGLE UNIT IS ALWAYS RADIANS.)
C
C        BARY   LOGICAL FLAG DEFINING OUTPUT CENTER.
C               ONLY THE 9 PLANETS ARE AFFECTED.
C                        BARY = .TRUE. =\ CENTER IS SOLAR-SYSTEM BARYCENTER
C                             = .FALSE. =\ CENTER IS SUN
C               DEFAULT VALUE = .FALSE.
C
C       PVSUN   DP 6-WORD ARRAY CONTAINING THE BARYCENTRIC POSITION AND
C               VELOCITY OF THE SUN.
C
C
      IMPLICIT DOUBLE PRECISION (A-H,O-Z)

      SAVE

      DIMENSION ET2(2),PV(6,12),PNUT(4),T(2),PJD(4),BUF(1500),
     . SS(3),CVAL(400),PVSUN(6)

      INTEGER LIST(12),IPT(3,13)

      LOGICAL FIRST
      DATA FIRST/.TRUE./

      CHARACTER*6 TTL(14,3),CNAM(400)
      CHARACTER*80 NAMFIL

      LOGICAL KM,BARY

      COMMON/EPHHDR/CVAL,SS,AU,EMRAT,NUMDE,NCON,IPT
      COMMON/CHRHDR/CNAM,TTL
      COMMON/STCOMX/KM,BARY,PVSUN

C
C       ENTRY POINT - 1ST TIME IN, GET POINTER DATA, ETC., FROM EPH FILE
C
      IF(FIRST) THEN
        FIRST=.FALSE.

C ************************************************************************
C ************************************************************************

C THE USER MUST SELECT ONE OF THE FOLLOWING BY DELETING THE 'C' IN COLUMN 1

C ************************************************************************

C        CALL FSIZER1(NRECL,KSIZE,NRFILE,NAMFIL)
        CALL FSIZER2(NRECL,KSIZE,NRFILE,NAMFIL)
C		 CALL FSIZER3(NRECL,KSIZE,NRFILE,NAMFIL)

      IF(NRECL .EQ. 0) WRITE(*,*)'  ***** FSIZER IS NOT WORKING *****'

C ************************************************************************
C ************************************************************************

      IRECSZ=NRECL*KSIZE
      NCOEFFS=KSIZE/2

        OPEN(NRFILE,
     *       FILE=NAMFIL,
     *       ACCESS='DIRECT',
     *       FORM='UNFORMATTED',
     *       RECL=IRECSZ,
     *       STATUS='OLD')

      READ(NRFILE,REC=1)TTL,CNAM,SS,NCON,AU,EMRAT,
     . ((IPT(I,J),I=1,3),J=1,12),NUMDE,(IPT(I,13),I=1,3)

      READ(NRFILE,REC=2)CVAL

      NRL=0

      ENDIF


C       ********** MAIN ENTRY POINT **********


      IF(ET2(1) .EQ. 0.D0) RETURN

      S=ET2(1)-.5D0
      CALL SPLIT(S,PJD(1))
      CALL SPLIT(ET2(2),PJD(3))
      PJD(1)=PJD(1)+PJD(3)+.5D0
      PJD(2)=PJD(2)+PJD(4)
      CALL SPLIT(PJD(2),PJD(3))
      PJD(1)=PJD(1)+PJD(3)

C       ERROR RETURN FOR EPOCH OUT OF RANGE

      IF(PJD(1)+PJD(4).LT.SS(1) .OR. PJD(1)+PJD(4).GT.SS(2)) GO TO 98

C       CALCULATE RECORD # AND RELATIVE TIME IN INTERVAL

      NR=IDINT((PJD(1)-SS(1))/SS(3))+3
      IF(PJD(1).EQ.SS(2)) NR=NR-1

        tmp1 = DBLE(NR-3)*SS(3) + SS(1)
        tmp2 = PJD(1) - tmp1
        T(1) = (tmp2 + PJD(4))/SS(3)

C       READ CORRECT RECORD IF NOT IN CORE

      IF(NR.NE.NRL) THEN
        NRL=NR
        READ(NRFILE,REC=NR,ERR=99)(BUF(K),K=1,NCOEFFS)
      ENDIF

      IF(KM) THEN
      T(2)=SS(3)*86400.D0
      AUFAC=1.D0
      ELSE
      T(2)=SS(3)
      AUFAC=1.D0/AU
      ENDIF

C   INTERPOLATE SSBARY SUN

      CALL INTERP(BUF(IPT(1,11)),T,IPT(2,11),3,IPT(3,11),2,PVSUN)

      DO I=1,6
      PVSUN(I)=PVSUN(I)*AUFAC
      ENDDO

C   CHECK AND INTERPOLATE WHICHEVER BODIES ARE REQUESTED

      DO 4 I=1,10
      IF(LIST(I).EQ.0) GO TO 4

      CALL INTERP(BUF(IPT(1,I)),T,IPT(2,I),3,IPT(3,I),
     & LIST(I),PV(1,I))

      DO J=1,6
       IF(I.LE.9 .AND. .NOT.BARY) THEN
       PV(J,I)=PV(J,I)*AUFAC-PVSUN(J)
       ELSE
       PV(J,I)=PV(J,I)*AUFAC
       ENDIF
      ENDDO

   4  CONTINUE

C       DO NUTATIONS IF REQUESTED (AND IF ON FILE)

      IF(LIST(11).GT.0 .AND. IPT(2,12).GT.0)
     * CALL INTERP(BUF(IPT(1,12)),T,IPT(2,12),2,IPT(3,12),
     * LIST(11),PNUT)

C       GET LIBRATIONS IF REQUESTED (AND IF ON FILE)

      IF(LIST(12).GT.0 .AND. IPT(2,13).GT.0)
     * CALL INTERP(BUF(IPT(1,13)),T,IPT(2,13),3,IPT(3,13),
     * LIST(12),PV(1,11))

      RETURN

  98  WRITE(*,198)ET2(1)+ET2(2),SS(1),SS(2)
 198  format(' ***  Requested JED,',f12.2,
     * ' not within ephemeris limits,',2f12.2,'  ***')

      stop

   99 WRITE(*,'(2F12.2,A80)')ET2,'ERROR RETURN IN STATE'

      STOP

      END
C+++++++++++++++++++++++++++++
C
      SUBROUTINE CONST(NAM,VAL,SSS,N)
C
C+++++++++++++++++++++++++++++
C
C     THIS ENTRY OBTAINS THE CONSTANTS FROM THE EPHEMERIS FILE
C
C     CALLING SEQEUNCE PARAMETERS (ALL OUTPUT):
C
C       NAM = CHARACTER*6 ARRAY OF CONSTANT NAMES
C
C       VAL = D.P. ARRAY OF VALUES OF CONSTANTS
C
C       SSS = D.P. JD START, JD STOP, STEP OF EPHEMERIS
C
C         N = INTEGER NUMBER OF ENTRIES IN 'NAM' AND 'VAL' ARRAYS
C
      IMPLICIT DOUBLE PRECISION (A-H,O-Z)

      SAVE

      CHARACTER*6 NAM(*),TTL(14,3),CNAM(400)

      DOUBLE PRECISION VAL(*),SSS(3),SS(3),CVAL(400),zips(2)
      DOUBLE PRECISION xx(99)
      data zips/2*0.d0/

      INTEGER IPT(3,13),DENUM,list(11)
      logical first
      data first/.true./

      COMMON/EPHHDR/CVAL,SS,AU,EMRAT,DENUM,NCON,IPT
      COMMON/CHRHDR/CNAM,TTL

C  CALL STATE TO INITIALIZE THE EPHEMERIS AND READ IN THE CONSTANTS

      IF(FIRST) CALL STATE(zips,list,xx,xx)
      first=.false.

      N=NCON

      DO I=1,3
      SSS(I)=SS(I)
      ENDDO

      DO I=1,N
      NAM(I)=CNAM(I)
      VAL(I)=CVAL(I)
      ENDDO

      RETURN

      END
